Other
Scientific paper
Jul 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993metic..28..374j&link_type=abstract
Meteoritics, vol. 28, no. 3, volume 28, page 374
Other
1
Antimony, Arsenic, Barringerite, Iron Meteorites, Metal, Partitioning, Experimental, Schreibersite, Troilite
Scientific paper
We have performed a series of experiments to evaluate the behaviors of As and Sb in metallic systems. Because of the reputed chalcophile nature of these elements, we wrongly anticipated that they would follow S and that, compared to the Fe-X systems [1], (solid metal/liquid metal) partition coefficients would be considerably lower in S-bearing systems. Experimental and Analytical: Experiments were performed in sealed silica tubes as in [2]. Starting materials were high-purity metals, natural pyrite, and natural stibnite. Charges were doped either with As or Sb. Experiments were held at either 950 degrees C for six days or 1250 degrees C for three days. Typical experimental assemblages consisted either of taenite and coexisting Fe-Ni-S-X liquid (1250 degrees and 950 degrees C) or an assemblage of troilite, schreibersite, and Fe-Ni-S-P-X liquid (950 degrees C). The schreibersite-bearing, As-doped charge also contained barringerite (Fe,Ni)2P. Charges were mounted in epoxy, polished, and analyzed using a Cameca SX-50 electron microprobe and standard techniques. Results: Phases appeared homogeneous. Our results, along with partition coefficients inferred for the S-free system, are given in Table 1. Table 1 appears here in the hard copy. Discussion: Our results indicate that As behaves as a siderophile element at low temperatures, very analogous to Au. While the siderophility of Sb increases with decreasing temperature, it remains incompatible in solid metal. In this regard Sb is unique. Both As and Sb are very incompatible in troilite. Arsenic is weakly incompatible in schreibersite and strongly compatible in barringerite. Nickel shows no preference for either phosphide. Nickel partition coefficients for metal and schreibersite are similar to those measured previously [3]. On a lnD vs. ln(1-2 alpha X(S)) diagram [4], the data for Sb and As subparallel each other, indicating similar dependencies on S, despite their very different partition coefficients. Arsenic behaves similarly to P. The As and Sb partition coefficients for the S-free system, inferred for kamacite (alpha-iron) from the Fe-As and Fe-Sb phase diagrams [1], are probably not applicable to taenite (gamma-iron). Extrapolation of our data to zero S indicates that the taenite partition coefficients for As and Sb are likely to be much lower than for kamacite. In discussing the fractional crystallization of iron meteorites, Scott [5] originally grouped Au, As, Sb, and Co and assigned them a (solid metal/liquid metal) partition coefficient of about 0.4. This distinguished them from P, which was given a partition coefficient of 0.2. Given the strong decoupling of As and Sb in our experiments, the general coherence of As and Sb in iron meteorites [5] is surprising. To explore this further, we have derived a new equation for the slopes of LogEl vs. LogNi diagrams, which takes into account changes in D. References: [1] Moffatt W. G. (1986) Handbook of Binary Phase Diagrams, Genium. [2] Jones J. H. and Drake M. J. (1983) GCA, 47, 1199. [3] Jones J. H. et al. (1993) GCA, 57, 453-460. [4] Jones J. H. and Malvin D. J. (1990) Metall. Trans., 21B, 697-706. [5] Scott E. R. D. (1972) GCA, 36, 1205.
Casanova Ignacio
Houston Jones Jane
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